2017
DOI: 10.1016/j.apsusc.2016.07.055
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Facile preparation of Z-scheme WO 3 /g-C 3 N 4 composite photocatalyst with enhanced photocatalytic performance under visible light

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Cited by 336 publications
(72 citation statements)
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“…Therefore, it has stronger redox capability and meanwhile retained its respective visible light absorption feature. Many g-C 3 N 4 based Z-scheme heterojunctions have been reported (such as BiVO 4 /g-C 3 N 4 [32], MoS 2 /g-C 3 N 4 [33], BiOCl/g-C 3 N 4 [34], Ag 3 PO 4 /g-C 3 N 4 [35], WO 3 /g-C 3 N 4 [36], and so on). LaFeO3 (LF) possessed the bandgap of ∼2.36 eV, corresponding the absorption wavelength of about 525 nm [37].…”
Section: Introductionmentioning
confidence: 99%
“…Therefore, it has stronger redox capability and meanwhile retained its respective visible light absorption feature. Many g-C 3 N 4 based Z-scheme heterojunctions have been reported (such as BiVO 4 /g-C 3 N 4 [32], MoS 2 /g-C 3 N 4 [33], BiOCl/g-C 3 N 4 [34], Ag 3 PO 4 /g-C 3 N 4 [35], WO 3 /g-C 3 N 4 [36], and so on). LaFeO3 (LF) possessed the bandgap of ∼2.36 eV, corresponding the absorption wavelength of about 525 nm [37].…”
Section: Introductionmentioning
confidence: 99%
“…However, the photocatalytic activity of pristine WO 3 is not high enough for practical use. Therefore, different strategies have been developed to increase the photocatalytic activity of WO 3 , including the preparation of WO 3 with different nanostructures [ 23 ], supporting noble metal Pt/Au/Ag [ 24 , 25 , 26 ], composites with other materials [ 27 , 28 , 29 ], and oxygen vacancy defects [ 30 , 31 , 32 , 33 , 34 ]. The introduction of oxygen vacancies is a simple and efficient strategy to improve the photocatalytic performance of WO 3 and it can greatly increase its conductivity and the absorption of visible light by local surface plasmon resonance (LSPR) in the near-infrared region, yielding an intensity that is comparable to bandgap absorption [ 35 , 36 ].…”
Section: Introductionmentioning
confidence: 99%
“…Since this first report, many investigations and characterizations have been published with differing XPS results. [77][78][79][80][81][82][83][84][85][86][87][88][89][90][91][92][93] Selected data are summarized in Ta ble S4 (Supporting Information), giving the binding energies for the C1sa nd N1ss ignals. Intriguingly, in most spectra,t he signal of C1sa ta round2 88 eV dominates the C1sr egion, but there are also spectra in which this peak exhibits the lowest intensity.T he most intense N1ss ignal ranges from 398.0 to 400.06eV ( Table S4).…”
Section: X-ray Photoelectron Spectroscopy Analysismentioning
confidence: 99%